Citing the Archive With Digial Object Identifiers (DOI)
The archive provides Digital Object Identifiers, or DOIs, for authors to use in their published works for citation purposes. A DOI provides a persistent and standardized link to the archive data and services that enabled an author's research.
For additional information on using DOIs, consult the DOI Wikipedia page and the DOI Handbook.
To request a new DOI for an archive data set or service, please submit a Helpdesk ticket.
| Resource Name | Description | Data Type | DOI |
|---|---|---|---|
| Confirmed Planets Table | The Confirmed Planets table contains physical and orbital parameters for the planet and the host star, as available from the default literature reference for each planet. | Dataset | 10.26133/NEA1 |
| Composite Planet Data Table | The Composite Planet Data table provides a collection of stellar an d planetary parameters for confirmed exoplanets, one row per planet. The table automatically selects the data from other available literature references for the same planet to fill in gaps from the default literature reference. | Dataset | 10.26133/NEA2 |
| K2 Candidates Table | The K2 candidates table lists objects from the published literature identified as candidates or false positives. If objects are confirmed as planets, their status in this table is updated but the objects remain. | Dataset | 10.26133/NEA3 |
| Kepler Objects of Interest (KOI) Cumulative Table | The Kepler Objects of Interest (KOI) Cumulative table gathers information from the individual KOI activity tables that describe the current results of different searches of the Kepler light curves. The intent of the cumulative table is to provide the most accurate dispositions and stellar and planetary information for all KOIs in one place. All the information in this table has provenance in other KOI activity tables. | Dataset | 10.26133/NEA4 |
| Kepler Objects of Interest DR25 Table | The Q1–Q17 Data Release 25 (DR25) Supplemental Kepler Objects-of-Interest (KOI) activity table reports dispositions based on the final processing (DR25) of the Kepler data and a combination of automated and human-based vetting to produce a "best-knowledge" catalog of planetary CANDIDATEs and FALSE POSITIVEs for use by the Astronomical community in selecting KOIs for follow-up observations and further study. | Dataset | 10.26133/NEA5 |
| Kepler Stellar Properties Table | The Kepler Stellar interactive table contains parameters for all targets observed by Kepler for the purpose of finding transiting planets. Individual tables include the values used for that specific processing, including the Q1–12, Q1–16, Q1–17 DR24, and Q1–17 DR25 pipeline runs. One additional table, the Q1–17 DR25 Supplemental Stellar, includes values provided by the Kepler Stellar Properties Working Group (SPWG) independent of any pipeline processing in order to report their most current stellar values. | Dataset | 10.26133/NEA6 |
| UKIRT Microlensing Survey | Light curves from the ongoing UKIRT microlensing survey made available with help from the UKIRT Microlensing Team. The Wide Field Camera (WFCAM) on the United Kingdom Infrared Telescope (UKIRT), located at Mauna Kea Observatory, has been used to conduct microlensing surveys with a variety of science goals. | Dataset | 10.26133/NEA7 |
| KELT Survey Light Curves | The Kilodegree Extremely Little Telescope (KELT) survey consists of two robotic telescopes that are conducting a survey for transiting exoplanets around bright stars. The NASA Exoplanet Archive currently contains about 1.1 million light curves in selected Northern fields. | Dataset | 10.26133/NEA8 |
| SuperWASP Survey Light Curves | SuperWASP consists of two robotic observatories that operate continuously throughout the year, allowing coverage of both hemispheres of the sky. The first, SuperWASP-North, is located on the island of La Palma among the Isaac Newton Group (ING) of telescopes. The second, SuperWASP-South, is located at the site of the South African Astronomical Observatory (SAAO), just outside Sutherland, South Africa. The NASA Exoplanet Archive hosts over 18 million light curves collected between 2004 and 2008. | Dataset | 10.26133/NEA9 |
| Transmission Spectroscopy Table | The transmission spectroscopy table contains wavelength-dependent transit measurements from the published literature. The transit measurements are published as either transit depths, planet-to-star radius ratios, or planet radii, and span wavelengths 0.3–24 microns. | Dataset | 10.26133/NEA11 |
| Emission Spectroscopy Table | The emission spectroscopy table contains wavelength-dependent eclipse measurements from the published literature. The eclipse measurements are published as either eclipse depths or brightness temperature, and span wavelengths 0.65–24 microns. | Dataset | 10.26133/NEA11 |
| Exoplanet Follow-up Observing Program—Kepler | The Exoplanet Follow-up Observing Program (ExoFOP) website is designed to optimize resources and facilitate collaboration in follow-up studies of exoplanet candidates. ExoFOP-Kepler serves as a repository for community-gathered follow-up data on Kepler planet candidates by allowing upload and display of data and derived astrophysical parameters. | Service | 10.26134/ExoFOP1 |
| Exoplanet Follow-up Observing Program—K2 | The Exoplanet Follow-up Observing Program (ExoFOP) website is designed to optimize resources and facilitate collaboration in follow-up studies of exoplanet candidates. ExoFOP-K2 serves as a repository for community-gathered follow-up data on K2 planet candidates by allowing upload and display of data and derived astrophysical parameters. |
Service | 10.26134/ExoFOP2 |
| Exoplanet Follow-up Observing Program—TESS | The Exoplanet Follow-up Observing Program (ExoFOP) website is designed to optimize resources and facilitate collaboration in follow-up studies of exoplanet candidates. ExoFOP-TESS serves as a repository for community-gathered follow-up data on TESS (Transiting Exoplanet Survey Satellite) planet candidates by allowing upload and display of data and derived astrophysical parameters. | Service | 10.26134/ExoFOP3 |
Last updated: 5 June 2019
